30 Jun 2025

Angular Momentum, Spin and Symmetry

Angular-momentum algebra, Pauli spinors, central fields, Clebsch-Gordan coupling, conservation laws, parity, identical particles, and spin-orbit coupling.

mj-18 angular-momentum electron-spin clebsch-gordan spin-orbit-coupling parity

Angular momentum is the generator of rotations. Its components satisfy

\[[J_i,J_j]=i\hbar\epsilon_{ijk}J_k, \qquad [J^2,J_i]=0.\]

Choose simultaneous eigenvectors of $J^2$ and $J_z$:

\[J^2\lvert jm\rangle=\hbar^2j(j+1)\lvert jm\rangle, \qquad J_z\lvert jm\rangle=\hbar m\lvert jm\rangle.\]

Eigenvalues from ladder operators

Define $J_\pm=J_x\pm iJ_y$. The commutators give

\[[J_z,J_\pm]=\pm\hbar J_\pm,\]

so $J_\pm\lvert jm\rangle$ has magnetic quantum number $m\pm1$. Also

\[J_-J_+=J^2-J_z^2-\hbar J_z, \qquad J_+J_-=J^2-J_z^2+\hbar J_z.\]

Taking norms,

\[\left\lVert J_+\lvert jm\rangle\right\rVert^2 =\hbar^2[j(j+1)-m(m+1)]\ge0,\] \[\left\lVert J_-\lvert jm\rangle\right\rVert^2 =\hbar^2[j(j+1)-m(m-1)]\ge0.\]

A finite ladder has a top $m_{\max}$ annihilated by $J_+$ and a bottom $m_{\min}$ annihilated by $J_-$. Hence

\[j(j+1)=m_{\max}(m_{\max}+1) =m_{\min}(m_{\min}-1),\]

which gives $m_{\max}=j$, $m_{\min}=-j$, and $2j\in{0,1,2,\ldots}$. Therefore

\[\boxed{j=0,\frac12,1,\frac32,\ldots, \qquad m=-j,-j+1,\ldots,j,}\] \[\boxed{ J_\pm\lvert jm\rangle =\hbar\sqrt{j(j+1)-m(m\pm1)}\,\lvert j,m\pm1\rangle. }\]

Electron spin and Pauli matrices

For spin $1/2$, $\mathbf S=(\hbar/2)\boldsymbol\sigma$, where

\[\sigma_x=\begin{pmatrix}0&1\\1&0\end{pmatrix},\quad \sigma_y=\begin{pmatrix}0&-i\\i&0\end{pmatrix},\quad \sigma_z=\begin{pmatrix}1&0\\0&-1\end{pmatrix}.\]

They obey

\[\sigma_i\sigma_j=\delta_{ij}I+i\epsilon_{ijk}\sigma_k, \qquad [S_i,S_j]=i\hbar\epsilon_{ijk}S_k.\]

The $S_z$ eigenvectors are

\[\lvert +z\rangle=\begin{pmatrix}1\\0\end{pmatrix}, \qquad \lvert -z\rangle=\begin{pmatrix}0\\1\end{pmatrix},\]

with eigenvalues $\pm\hbar/2$. The normalized eigenvectors of $S_x$ are

\[\lvert\pm x\rangle=\frac1{\sqrt2} \begin{pmatrix}1\\\pm1\end{pmatrix},\]

and those of $S_y$ are

\[\lvert\pm y\rangle=\frac1{\sqrt2} \begin{pmatrix}1\\\pm i\end{pmatrix}.\]

Motion in a centrally symmetric field

For

\[H=\frac{\mathbf p^2}{2\mu}+V(r),\]

rotational symmetry gives $[H,\mathbf L]=0$ and $[H,L^2]=0$. For $\psi(\mathbf r)=R_l(r)Y_l^m(\theta,\phi)$, the spherical Laplacian gives

\[\nabla^2(R_lY_l^m) =\left[ \frac1{r^2}\frac d{dr}\left(r^2\frac{dR_l}{dr}\right) -\frac{l(l+1)}{r^2}R_l \right]Y_l^m.\]

Set $u_l=rR_l$. Since

\[r^2\frac{dR_l}{dr}=ru_l^{\prime}-u_l, \qquad \frac1{r^2}\frac d{dr}(ru_l^{\prime}-u_l)=\frac{u_l^{\prime\prime}}{r},\]

division of the Schrödinger equation by $Y_l^m/r$ gives

\[\boxed{ -\frac{\hbar^2}{2\mu}\frac{d^2u_l}{dr^2} +\left[V(r)+\frac{\hbar^2l(l+1)}{2\mu r^2}\right]u_l=Eu_l. }\]

For a nonsingular bound-state solution, $u_l(0)=0$; normalizability requires $u_l(r)\to0$ as $r\to\infty$. The central potential makes the energy independent of $m$.

Addition of angular momenta

For $\mathbf J=\mathbf J_1+\mathbf J_2$, the uncoupled and coupled bases are related by Clebsch-Gordan coefficients:

\[\lvert jm\rangle =\sum_{m_1,m_2} \lvert j_1m_1\rangle\lvert j_2m_2\rangle \langle j_1m_1;j_2m_2\mid jm\rangle.\]

Since $J_z=J_{1z}+J_{2z}$, a coefficient can be nonzero only if $m=m_1+m_2$. Ladder termination gives the angular-momentum selection rule

\[\boxed{\lvert j_1-j_2\rvert\le j\le j_1+j_2}\]

in integer steps. For two spin-$1/2$ particles,

\[\lvert1,1\rangle=\lvert++\rangle, \qquad \lvert1,0\rangle=\frac{\lvert+-\rangle+\lvert-+\rangle}{\sqrt2},\] \[\lvert1,-1\rangle=\lvert--\rangle, \qquad \lvert0,0\rangle=\frac{\lvert+-\rangle-\lvert-+\rangle}{\sqrt2}.\]

The triplet is symmetric under particle exchange; the singlet is antisymmetric.

Space-time symmetries and conservation laws

An infinitesimal continuous transformation generated by $G$ is $U(\varepsilon)=I-i\varepsilon G/\hbar$. If the Hamiltonian is invariant, $UHU^\dagger=H$, then to first order

\[H-\frac{i\varepsilon}{\hbar}[G,H]=H \quad\Longrightarrow\quad [G,H]=0.\]

The Heisenberg equation then gives $d\langle G\rangle/dt=0$. Spatial translations are generated by $\mathbf P$, rotations by $\mathbf J$, and time translations by $H$ itself. Their invariance therefore conserves linear momentum, angular momentum, and energy, respectively.

Parity is the discrete inversion

\[\Pi\psi(\mathbf r)=\psi(-\mathbf r), \qquad \Pi^2=I.\]

Its eigenvalues are $\pm1$. For a parity-even Hamiltonian, $[H,\Pi]=0$, so parity is conserved. Central-field states have parity $(-1)^l$ because $Y_l^m(-\hat{\mathbf r})=(-1)^lY_l^m(\hat{\mathbf r})$.

Exclusion, exchange symmetry, and spin-orbit coupling

For identical particles, exchanging labels cannot change any observable. For distinct orthonormal one-particle orbitals $\phi_a$ and $\phi_b$, the normalized symmetric and antisymmetric combinations are

\[\Psi_\pm(1,2)=\frac1{\sqrt2} [\phi_a(1)\phi_b(2)\pm\phi_b(1)\phi_a(2)].\]

Electrons are fermions, so the complete state must be antisymmetric. If the two orbital labels coincide, applying the antisymmetrizer gives zero rather than a normalizable state; the symmetric product is simply $\phi_a(1)\phi_a(2)$. Thus no two electrons may occupy the same complete one-particle state. A symmetric spin triplet must accompany an antisymmetric spatial state, while the antisymmetric spin singlet accompanies a symmetric spatial state.

With electron spin $s=1/2$, total angular momentum is $\mathbf J=\mathbf L+\mathbf S$. The identity

\[J^2=L^2+S^2+2\mathbf L\cdot\mathbf S\]

gives

\[\boxed{ \mathbf L\cdot\mathbf S\,\lvert lsjm\rangle =\frac{\hbar^2}{2} [j(j+1)-l(l+1)-s(s+1)]\lvert lsjm\rangle. }\]

For $l>0$, the allowed values are $j=l\pm1/2$. Therefore

\[\langle\mathbf L\cdot\mathbf S\rangle =\begin{cases} (\hbar^2/2)l,&j=l+1/2,\\ -(\hbar^2/2)(l+1),&j=l-1/2. \end{cases}\]

For an electron moving in a central potential energy $V(r)$, the nonrelativistic spin-orbit interaction, including the Thomas factor, is

\[\boxed{ H_{SO}=\frac1{2m_e^2c^2r}\frac{dV}{dr}\, \mathbf L\cdot\mathbf S. }\]

It consequently splits a fixed $l$ level into the two allowed total-angular-momentum levels $j=l\pm1/2$.

For a fixed radial state, define the radial expectation

\[\boxed{ \xi_{nl}=\left\langle nl\right\lvert \frac1{2m_e^2c^2r}\frac{dV}{dr} \left\lvert nl\right\rangle. }\]

The first-order spin-orbit shift is therefore

\[\boxed{ \Delta E_{nlj} =\frac{\xi_{nl}\hbar^2}{2} [j(j+1)-l(l+1)-s(s+1)]. }\]

The level ordering in the figure assumes $\xi_{n1}>0$; a negative radial expectation reverses the two levels.

Equation-generated spin-orbit splitting of an l equals one level into j equals three halves and one half
For \(l=1\) and \(\xi_{n1}>0\), \(\langle\mathbf L\cdot\mathbf S\rangle/\hbar^2=1/2\) for \(j=3/2\) and \(-1\) for \(j=1/2\); the ordering reverses when \(\xi_{n1}<0\).

Solved Problems

1. Spin components from a normalized Pauli spinor

For

\[\lvert\psi\rangle= \begin{pmatrix}\sqrt3/2\\i/2\end{pmatrix},\]

normalization follows from $3/4+1/4=1$. A measurement of $S_z$ gives $+\hbar/2$ with probability $3/4$ and $-\hbar/2$ with probability $1/4$. Hence

\[\langle S_z\rangle =\frac\hbar2\left(\frac34-\frac14\right)=\frac\hbar4.\]

For the other components,

\[\langle S_i\rangle=\frac\hbar2 \langle\psi\rvert\sigma_i\lvert\psi\rangle.\]

Direct matrix multiplication gives

\[\langle\sigma_x\rangle=0, \qquad \langle\sigma_y\rangle=\frac{\sqrt3}{2}, \qquad \langle\sigma_z\rangle=\frac12,\]

so

\[\boxed{ \langle\mathbf S\rangle =\left(0,\frac{\sqrt3\hbar}{4},\frac\hbar4\right), \qquad \left\lvert\langle\mathbf S\rangle\right\rvert=\frac\hbar2.}\]

Every component has units of angular momentum. The maximal magnitude $\hbar/2$ shows that this pure spinor points along the unit direction $(0,\sqrt3/2,1/2)$.

2. Regular radial behavior at the origin

Suppose $V(r)$ remains finite at $r=0$. Near the origin the centrifugal term dominates the radial equation for $l>0$:

\[-\frac{\hbar^2}{2\mu}u_l^{\prime\prime} +\frac{\hbar^2l(l+1)}{2\mu r^2}u_l\simeq0.\]

With $u_l\sim r^p$, cancellation of the common factor $r^{p-2}$ gives

\[p(p-1)-l(l+1)=0,\]

whose roots are $p=l+1$ and $p=-l$. For $l=2$,

\[u_2(r)\sim C_1r^3+C_2r^{-2}.\]

Because the radial norm is $\int_0^\infty\lvert u_l(r)\rvert^2dr$, the $r^{-2}$ branch produces a divergent integral at the origin. Therefore

\[\boxed{u_2(r)\propto r^3, \qquad R_2(r)=u_2(r)/r\propto r^2\quad(r\to0).}\]

The coefficient carries the units needed by the normalization; the power law itself is independent of the particle mass and of the finite value $V(0)$.

3. Coupling $l=1$ to spin $1/2$

The unique state with maximum $m$ is

\[\left\lvert\frac32,\frac32\right\rangle =\lvert1,1\rangle\left\lvert\frac12,\frac12\right\rangle.\]

Apply $J_-=L_-+S_-$. On the coupled state,

\[J_-\left\lvert\frac32,\frac32\right\rangle =\hbar\sqrt3\left\lvert\frac32,\frac12\right\rangle.\]

On the uncoupled product,

\[(L_-+S_-)\lvert1,1\rangle\lvert+\rangle =\hbar\sqrt2\lvert1,0\rangle\lvert+\rangle +\hbar\lvert1,1\rangle\lvert-\rangle.\]

Dividing by $\hbar\sqrt3$ gives

\[\boxed{ \left\lvert\frac32,\frac12\right\rangle =\sqrt{\frac23}\lvert1,0\rangle\lvert+\rangle +\sqrt{\frac13}\lvert1,1\rangle\lvert-\rangle.}\]

The normalized orthogonal combination with the same total $m=1/2$ is

\[\boxed{ \left\lvert\frac12,\frac12\right\rangle =\sqrt{\frac13}\lvert1,0\rangle\lvert+\rangle -\sqrt{\frac23}\lvert1,1\rangle\lvert-\rangle.}\]

The squared coefficients in either line add to one, and every product ket has $m_l+m_s=1/2$, providing normalization and selection-rule checks.

Descriptive Questions

  1. Starting from the angular-momentum commutators, derive the allowed values of $j$ and $m$ and the normalized action of $J_\pm$.
  2. Derive the radial Schrödinger equation for a central potential, stating both endpoint boundary conditions and the origin of the centrifugal term.
  3. Explain how translation, rotation, time-translation, and parity invariance lead to their corresponding conservation laws, noting why parity is a discrete symmetry.
  4. For two identical electrons, relate exchange symmetry of the spatial and spin factors to the exclusion principle and to the singlet-triplet classification.

Numerical Problems

  1. For $j=5/2$ and $m=-3/2$, find the eigenvalues of $J^2$ and $J_z$ and the magnitude $\sqrt{\langle J^2\rangle}$.
  2. Evaluate $J_+\lvert2,-1\rangle$, including its numerical coefficient and final magnetic quantum number.
  3. Find the centrifugal energy $\hbar^2l(l+1)/(2m_er^2)$ for an electron with $l=2$ at $r=0.200\,\mathrm{nm}$. Use $\hbar^2/(2m_e)=3.80998\,\mathrm{eV\,\mathring A^2}$.
  4. Couple $j_1=3/2$ and $j_2=1$. List all allowed $j$ values and verify the number of product states from the dimensions of the coupled multiplets.
  5. For $l=3$, $s=1/2$, and $\xi_{nl}\hbar^2=0.800\,\mathrm{meV}$, calculate both spin-orbit shifts and their separation.
  6. Two normalized one-particle orbitals have real overlap $S=1/3$. Find the normalization constants multiplying $\phi_a(1)\phi_b(2)\pm\phi_b(1)\phi_a(2)$.

Final answers: 1. $J^2=35\hbar^2/4$, $J_z=-3\hbar/2$, magnitude $\sqrt{35}\hbar/2$; 2. $J_+\lvert2,-1\rangle=\sqrt6\hbar\lvert2,0\rangle$; 3. $5.71497\,\mathrm{eV}$; 4. $j=1/2,3/2,5/2$ and $2+4+6=12=(2j_1+1)(2j_2+1)$; 5. $+1.200\,\mathrm{meV}$ for $j=7/2$, $-1.600\,\mathrm{meV}$ for $j=5/2$, separation $2.800\,\mathrm{meV}$; 6. $N_+=3/\sqrt{20}$ and $N_-=3/4$.

The core derivations and all problem answers are verified in the original Maxima worksheet and the problems worksheet; every printed residual is zero.

References

  1. Angular momentum operator.
  2. J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Chapters 3, 4, and 7.
  3. D. J. Griffiths and D. F. Schroeter, Introduction to Quantum Mechanics, 3rd ed., Chapters 4 and 5.
© Rajesh Kumar, SKMU · Physics Lecture Notes · rajeshphy.github.io

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